On the other hand, an interacting DE model is discussed, on which we have performed a global fitting, by using an analysis combined of Joint Light Curve
Analysis (JLA) type Ia Supernovae (SNe Ia) data [1]}, [2]}, [3]}, including the growth rate of structure formation
obtained from redshift space distortion (RSD) data
[4]}, [5]}, [6]}, [7]}, [8]}, [9]}, [10]}, [11]}, [12]}, [13]}, [14]}, [15]}, [16]}, [17]}, [18]}, [19]}, [20]}, [21]}, [22]}, [23]},
together with Baryon Acoustic Oscillation (BAO) data
[24]}, [25]}, [26]}, [27]}, [28]}, [29]}, [30]}, [31]}, [32]}, [33]}, [34]}, [35]}, [36]}, [37]}, [38]},
as well as the observations of anisotropies in the power spectrum of the Cosmic Microwave Background (CMB) data
[23]}, [40]}, [41]}, [42]} and the Hubble parameter (H) data obtained from galaxy
surveys [43]}, [44]}, [45]}, [46]}, [47]}, [48]}, [49]}, [50]}, [51]}, [52]} to constrain the
parameter space of such model and break the degeneracy of their parameters, putting tighter constraints on them.
